Relativistic magnetosonic solitons with reflected particles in electron–positron plasmas
Phys. Fluids 31, 839 (1988); doi:10.1063/1.866765
Issue Date: April 1988
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The presence of magnetically reflected particles is shown to allow the existence of large amplitude magnetosonic solitary waves in relativistic electron–positron plasmas. If the flow is assumed to contain a single loop of gyrating particles, self-consistent structures are found with peak field amplitudes (B/B
)max<(11)1/2, where B
is the magnitude of the upstream magnetic field. In contrast, without reflected particles, the amplitude of a relativistic magnetosonic soliton is restricted to (B/B
) −1<2/
, where 
is the upstream Lorentz factor. Therefore, if 
![[infinity]](http://scitation.aip.org/stockgif3/infin-script.gif)
1, reflected particles greatly increase the allowable amplitudes of these nonlinear waves. It is also shown that when 
![[infinity]](http://scitation.aip.org/stockgif3/infin-script.gif)
1, the wave properties are independent of 
, and are completely parametrized by the ratio of the Poynting flux to the kinetic energy flux in the upstream flow. Some new features of solitary waves without reflected particles are also derived, and a heuristic model is presented which gives a simple physical interpretation of many of these results.
Physics of Fluids is copyrighted by The American Institute of Physics.
)max<(11)1/2, where B
is the magnitude of the upstream magnetic field. In contrast, without reflected particles, the amplitude of a relativistic magnetosonic soliton is restricted to (B/B
) −1<2/
, where 
is the upstream Lorentz factor. Therefore, if 
![[infinity]](http://scitation.aip.org/stockgif3/infin-script.gif)
1, reflected particles greatly increase the allowable amplitudes of these nonlinear waves. It is also shown that when 
![[infinity]](http://scitation.aip.org/stockgif3/infin-script.gif)
1, the wave properties are independent of 
, and are completely parametrized by the ratio of the Poynting flux to the kinetic energy flux in the upstream flow. Some new features of solitary waves without reflected particles are also derived, and a heuristic model is presented which gives a simple physical interpretation of many of these results.
Physics of Fluids is copyrighted by The American Institute of Physics.
| History: | Received 20 August 1987; accepted 5 January 1988 |
| Permalink: | http://dx.doi.org/10.1063/1.866765 |
KEYWORDS and PACS
RELATIVISTIC PLASMA,
MAGNETOACOUSTIC WAVES,
SOLITONS,
ENERGY LOSSES,
ELECTRONS,
POSITRONS,
MAGNETIZATION,
ASTROPHYSICS,
AMPLITUDES,
REFLECTION,
KINETIC ENERGY,
COLLISIONLESS PLASMA,
SHOCK WAVES,
ENERGY LOSSES
- 52.35.Sb
The physics of plasmas and electric discharges Waves, oscillations, and instabilities in plasma Solitons; BGK modes - 52.35.Tc
The physics of plasmas and electric discharges Waves, oscillations, and instabilities in plasma Shock waves - 52.60.+h
The physics of plasmas and electric discharges Relativistic plasma - 95.30.Qd
Fundamental astronomy and astrophysics; instrumentation, techniques, and astronomical observations Fundamental aspects of astrophysics Hydromagnetics and plasmas - YEAR: 1988
RELATED DATABASES
PUBLICATION DATA
0031-9171 (print)
1089-7666 (online)
REFERENCES (15)
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